https://doi.org/10.1051/epjconf/201715205004
Asteroseismology of the Kepler target KIC 9204718
1 School of Aviation, Girne American University, University Drive, P.O. Box 5, 99428 Karmi Campus, Karaoğlanoğlu, Kyrenia, Turkey
2 College of Graduate Studies, University of South Africa, PO Box 392, Unisa, 0003 Pretoria, South Africa
3 Institute of Astronomy with NAO, Bulgarian Academy of Sciences, blvd. Tsarigradsko chaussee 72, Sofia 1784, Bulgaria
4 Izmir Turk College Planetarium, 8019/21 sok., No: 22, Izmir, Turkey
Published online: 8 September 2017
The high precision data obtained by the Kepler satellite allows us to detect hybrid-type pulsator candidates more accurately than the data obtained by ground–based observations. In this study, we present preliminary results on the new analysis of the Kepler light curve and high-resolution spectroscopic observations of the pulsating Am star KIC 9204718. Our tentative analysis shows that the star has hybrid-type pulsational characteristics.
© The Authors, published by EDP Sciences, 2017
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
